How does the lifespan of a star packing 100 solar masses compare to the potential lifetime of low-mass red dwarfs?
Answer
The 100 solar mass star endures for millions of years, while red dwarfs stretch into trillions
The disparity in lifespan based on initial mass is profound. Lower-mass stars, such as red dwarfs, consume their fuel incredibly slowly, resulting in lifetimes that can extend far beyond the current age of the universe, potentially reaching twelve trillion years. In stark contrast, a star with a mass of 100 solar masses burns its fuel furiously due to the immense core pressures required for equilibrium. This rapid consumption limits its total existence to a mere few million years, meaning it expires before the universe has even completed its first billion years of existence.

Related Questions
What five basic characteristics fundamentally describe every star in the universe?What contest does a star's mass set the stakes for concerning gravity and nuclear fusion pressure?How is stellar mass conventionally quantified relative to our Sun for calculation purposes?How does the lifespan of a star packing 100 solar masses compare to the potential lifetime of low-mass red dwarfs?What is the approximate diameter range for extremely compressed stellar remnants known as neutron stars?What two physical properties mathematically determine a star's total energy broadcast, known as luminosity?On what absolute temperature scale is stellar surface temperature quantified, setting absolute zero at 0 K?Which spectral class designation corresponds to the coolest M-class stars appearing distinctly red?What standardized measure defines a star’s true brightness by hypothetically placing it at a fixed distance of 10 parsecs?What relationship is plotted on the Hertzsprung-Russell diagram concerning temperature and brightness?